The Performance of TripleSpec at Palomar

被引：65

作者：

Herter, Terry L. ^{[1
]}

Henderson, Charles P. ^{[1
]}

Wilson, John C. ^{[2
]}

Matthews, Keith Y. ^{[3
]}

Rahmer, Gustavo ^{[3
]}

Bonati, Marco ^{[3
]}

Muirhead, Philip S. ^{[1
]}

Adams, Joseph D. ^{[1
]}

Lloyd, James P. ^{[1
]}

Skrutskie, Michael F. ^{[2
]}

Moon, Dae-Sik ^{[4
]}

Parshley, Stephen C. ^{[1
]}

Nelson, Matthew J. ^{[2
]}

Martinache, Frantz ^{[1
]}

Gull, George E. ^{[1
]}

机构：

[1] Cornell Univ, Space Sci Bldg, Ithaca, NY 14853 USA

[2] Univ Virginia, Charlottesville, VA 22903 USA

[3] CALTECH, Div Physi Math & Astron, Pasadena, CA 91125 USA

[4] Univ Toronto, Toronto, ON M5S 3H4, Canada

来源：

GROUND-BASED AND AIRBORNE INSTRUMENTATION FOR ASTRONOMY II, PTS 1-4 | 2008年 / 7014卷

关键词：

Near Infrared; Spectroscopy; Cross-Dispersed;

D O I：

10.1117/12.789660

中图分类号：

V [航空、航天];

学科分类号：

08 ; 0825 ;

摘要：

We report the performance of Triplespec from commissioning observations on the 200-inch Hale Telescope at Palomar Observatory. Triplespec is one of a set of three near-infrared, cross-dispersed spectrographs covering wavelengths from 1 - 2.4 microns simultaneously at a resolution of similar to 2700. At Palomar, Triplespec uses a 1x30 arcsecond slit. Triplespec will be used for a variety of scientific observations, including moderate to high redshift galaxies, star formation, and low mass stars and brown dwarfs. When used in conjunction with an externally dispersed interferometer, Triplespec will also detect and characterize extrasolar planets.

引用

页数：8

共 8 条

[1]

EDELSTEIN J, 2008, P SPIE, V7014

[2]

Gillett FC, 1998, ASTR SOC P, V133, P42

[3]

HERTER T, TRIPLESPEC R 2 UNPUB

[4] OBSERVATIONS OF THE OH AIRGLOW EMISSION [J].

MAIHARA, T ;

IWAMURO, F ;

YAMASHITA, T ;

HALL, DNB ;

COWIE, LL ;

TOKUNAGA, AT ;

PICKLES, A .

PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC, 1993, 105 (691) :940-944

[5]

Skrutskie MF, 1997, ASTROPHYS SPACE SC L, V210, P25, DOI 10.1007/978-94-011-5784-1_3

[6] The Spitzer Space Telescope mission [J].

Werner, MW ;

Roellig, TL ;

Low, FJ ;

Rieke, GH ;

Rieke, M ;

Hoffmann, WF ;

Young, E ;

Houck, JR ;

Brandl, B ;

Fazio, GG ;

Hora, JL ;

Gehrz, RD ;

Helou, G ;

Soifer, BT ;

Stauffer, J ;

Keene, J ;

Eisenhardt, P ;

Gallagher, D ;

Gautier, TN ;

Irace, W ;

Lawrence, CR ;

Simmons, L ;

Van Cleve, JE ;

Jura, M ;

Wright, EL ;

Cruikshank, DP .

ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 2004, 154 (01) :1-9

[7] 'Mass Producing' an efficient NIR spectrograph [J].

Wilson, JC ;

Henderson, CP ;

Herter, TL ;

Matthews, K ;

Skrutskie, MF ;

Adams, JD ;

Moon, DS ;

Smith, R ;

Gautier, N ;

Ressler, M ;

Soifer, BT ;

Lin, S ;

Howard, J ;

LaMarr, J ;

Stolberg, TM ;

Zink, J .

GROUND-BASED INSTRUMENTATION FOR ASTRONOMY, PTS 1-3, 2004, 5492 :1295-1305

[8] The Sloan Digital Sky Survey: Technical summary [J].

York, DG ;

Adelman, J ;

Anderson, JE ;

Anderson, SF ;

Annis, J ;

Bahcall, NA ;

Bakken, JA ;

Barkhouser, R ;

Bastian, S ;

Berman, E ;

Boroski, WN ;

Bracker, S ;

Briegel, C ;

Briggs, JW ;

Brinkmann, J ;

Brunner, R ;

Burles, S ;

Carey, L ;

Carr, MA ;

Castander, FJ ;

Chen, B ;

Colestock, PL ;

Connolly, AJ ;

Crocker, JH ;

Csabai, I ;

Czarapata, PC ;

Davis, JE ;

Doi, M ;

Dombeck, T ;

Eisenstein, D ;

Ellman, N ;

Elms, BR ;

Evans, ML ;

Fan, XH ;

Federwitz, GR ;

Fiscelli, L ;

Friedman, S ;

Frieman, JA ;

Fukugita, M ;

Gillespie, B ;

Gunn, JE ;

Gurbani, VK ;

de Haas, E ;

Haldeman, M ;

Harris, FH ;

Hayes, J ;

Heckman, TM ;

Hennessy, GS ;

Hindsley, RB ;

Holm, S .

ASTRONOMICAL JOURNAL, 2000, 120 (03) :1579-1587

← 1 →